GPI IFS Data Handbook¶
This document describes the GPI Integral Field Spectrograph (IFS), the properties of its output data, including various systematics and noise sources that one may encounter, and how these data should be calibrated. Its goal is to summarize in one place all the properties of GPI data that a new user should be familiar with to usefully work with the data.
See also the Pipeline User’s Guide, which describes the user interface and operation of the software used to process these data.
The Processing GPI Data, Step by Step section of this Handbook is particularly recommended to understand the details and potential pitfalls of each step of GPI data reduction.
Warning
This is a WORKING DRAFT document, which is not fully complete and may be in error in some places. It represents our current understanding of these aspects of instrument performance, and is likely to evolve with time. Use your own scientific judgement when reducing and analyzing data from GPI.
Read carefully, examine your data, evaluate the systematics, and let’s find some planets...
Contents¶
- GPI IFS Detector Properties
- Field of View and Lenslet Geometry
- Filters and Spectra
- GPI Data Formats
- Processing GPI Data, Step by Step
- Darks
- Thermal/Sky Backgrounds
- Bad Pixels
- Destriping and Microphonics
- Saturation and Nonlinearity
- Persistence
- Flat Fielding
- Flat Fielding: Lenslet Array Flat
- Wavelength Calibration
- IFS Flexure
- Datacube Extraction
- Satellite Spot Calibrations
- Astrometric Calibration and Distortion Correction
- Photometric Calibration
- PSF Subtractions
- Spectral Extraction of Companions
- Processing GPI Data, Step by Step: Polarimetry
- A Gallery of Example Data, Artifacts, and Noise Sources to be Aware Of